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Fig. B.1

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Stacked spectra with CASSIS model fits with Tex = 100 K for all species aside from NO which is modelled at 40 K. The grey region shows the +/- 1σ error. The vertical dashed lines denote the rest frequency of the lines. The CH3OH model is with a column density of 5 × 1014 cm−2. In Fig. 2 we show how a higher column density better fits weaker CH3OH lines covered in the observations.

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